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Table 5.
Dust heating mechanisms derived from both methods for each sample galaxy. “YS” = young stars; “ES” = evolved stars. AGN hosts are indicated by an asterisk (*).
| Galaxy name | Method 1 (r) | Method 2 (p-value) |
|---|---|---|
| NGC 300 | YS | YS |
| NGC 2403 | YS | YS |
| IC 342 | ES | ES |
| NGC 7793 | YS | YS |
| NGC 3031 (M 81) | ES | ES |
| NGC 6946 | ES | ES |
| NGC 4736 (M 94) | ES | ES |
| NGC 5236 (M 83) | ES | ES |
| NGC 3621* | YS | YS |
| NGC 5457 (M 101) | YS | ES |
| NGC 5194 (M 51)* | ES | ES |
| NGC 925 | YS | YS |
| NGC 628 (M 74) | YS | ES |
| NGC 5055 (M 63) | YS | ES |
| NGC 4725* | YS | ES |
| NGC 3521 | YS | ES |
| NGC 1097 | ES | ES |
| NGC 1365* | ES | ES |
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